By Stephen James O'Meara

Stephen O'Meara's new and intriguing watching consultant spotlights an unique choice of 109 deep-sky items that may attract sky-watchers around the world. His 'hidden treasures' comprise an excellent collection of galaxies, open clusters, planetary nebulae and extra, all of that have been conscientiously selected in accordance with their reputation and simplicity of watching. None of those items are integrated in both the Messier or the Caldwell catalogs, and all are seen in a 4-inch telescope lower than darkish skies. wonderful images and gorgeous drawings accompany exact visible descriptions of the items, which come with their wealthy histories and astrophysical importance. The author's unique finder charts are designed to aid observers get to their ambitions quickly and successfully.

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The cluster is in an oddball retrograde orbit traveling at a speed of about 305 kilometers per second some 39,000 lightyears from the Milky Way’s center. It’s a loose halo cluster whose members each contain, 1 1 on average, anywhere from 13 to 20 as much iron as does the Sun. That’s about the same abundance that each cluster member has in globular cluster NGC 1851 in Columba – a galactic veteran of 14 billion years. How old is NGC 288? Well, that has been the matter of debate for many years. Some researchers claimed it was the same age as another aged globular – NGC 362 in Tucana.

Compared to large and scattered NGC 225, NGC 189 is small and round. It also has a beautiful bluish cometlike sheen that stands out distinctly from the background, especially when seen together with NGC 225. NGC 189 lies immediately north of a 7 -wide trapezoid of four 9th- and 10th-magnitude suns. In photographs, the cluster resides within a comparatively rich region bordering the heavily obscured sack of dark nebulosity within which NGC 225 is located. A study of the region by George Alter reveals that the background density is, however, about half that of the other clusters in the neighborhood so that some absorption might justifiably be assumed.

Archinal suspects many more stars in the nebula may be associated with the cluster. Guillaume Bigourdan’s (1899–1917) discovery of IC 1590 was no less of an achievement than Barnard’s. It takes a certain visual perspicacity to go beyond what one is expected to see (a nebula) and to find something new within it. Bigourdan was a highly esteemed visual observer. He found about 100 new nebulae and clusters with the 12-inch refractor at Paris Observatory, France, and IC 1590 was one of them. xml CUUK347B-O’Meara September 29, 2006 9:32 3 of Technology) notes that Bigourdan’s position of the cluster is about 3 southeast of the obvious group of stars taken to be IC 1590.

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Deep-Sky Companions Hidden Treasures by Stephen James O'Meara


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